The accurate estimation of electron density in the ionosphere is crucial to serving various applications including remote sensing systems, communication, satellite positioning, and navigation, which would contribute to mitigating the adverse space weather effects. Due to the regular and irregular variations in the ionosphere, such as daily and seasonal variations, sporadic E, ionospheric storms, 11-year sunspot cycle, and so on, there are difficulties in the ionospheric models for electron density.In the past decades, the empirical and physical modeling approaches for ionosphere were widely used, including the International Reference Ionosphere (IRI), Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIE-GCM), Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP), Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM), and Ground to topside model of the Atmosphere and Ionosphere for Aeronomy (GAIA), etc. (D.